ABC’s National Science Week citizen science project Galaxy Explorer has been a huge success, with every single one of the 220,000 galaxies in GAMA batch classified by the minimum of five different users (to exclude inadvertent or malicious misclassification), for a total of over one million classifications!
Galaxy Explorer had 18,163 registered participants, which averages out at 55 galaxy classifications per user.
As at 27 August the highest number of classifications done by a single user was over 17,000, and the most for a school group was 12,000!
That single user figure is incredible, but let’s just hope they weren’t compromising quality in the pursuit of quantity!
As for me I classified 161 galaxies, so I’m content to be above-average 😉
NASA’s Cassini team has discovered a global ocean beneath the frozen surface of Saturn’s moon Enceladus.
Back in 2005 the Cassini spacecraft observed geysers jetting into space from the moon’s south pole, and scientists had more recently confirmed the presence of a sub-surface sea in that region. This discovery indicates that the ocean of liquid water encapsulates the moon’s rocky core.
The discovery is the result of analysis of years of imagery taken by the Cassini spacecraft. Scientists carefully mapped Enceladus’ surface features across hundreds of images in order to make extremely precise measurements of the moon’s rotation.
They observed the moon had a small wobble in its orbit around Saturn, called a libration. Models showed the libration’s characteristics could only be explained if the moon’s icy surface was not moving in sync with its rocky core (which comprises most of its mass), and therefore a moon-wide liquid ocean must be separating the two.
“This was a hard problem that required years of observations, and calculations involving a diverse collection of disciplines, but we are confident we finally got it right.” – Peter Thomas, Cornell University
Enceladus is one of a handful of bodies in the Solar System which are believed to have oceans of liquid water. Jupiter’s moon Europa is the best-known – scientists think it might have a large subsurface saltwater ocean beneath its icy crust, warmed by the giant planet’s gravity squeezing the moon, heating it in the process.
A free-moving liquid water ocean (as opposed to one where isolated pockets of water are sandwiched in between layers of ice) opens up the possibility that the moons could potentially support life (though whether life actually exists on Europa or Enceladus is extremely uncertain).
Jupiter’s large moons Ganymede and Callisto may also have trapped seas of liquid water, as may two more of Saturn’s Moons, Titan and Mimas, and the dwarf planet Ceres.
The Cassini mission launched from Cape Canaveral in October of 1997. It took nearly seven years to reach the Saturnian system, where it has been operating now for 11 years. In that time the truck-sized spacecraft has launched a European-made probe, named Huygens, which parachuted into Titan’s thick atmosphere, landing on the surface and capturing the first and only images from the huge moon’s surface.
Cassini has also taken measurements and imagery of Saturn and its dozens of moons, and even captured a sequel to Voyager 1’s famous ‘Pale Blue Dot‘ portrait of Earth:
NASA’s Cassini spacecraft has captures the majesty of Saturn’s rings and Earth (indicated by arrow) in the same frame. Credit: NASA/JPL-Caltech/Space Science Institute
Dramatic plumes, both large and small, spray water ice out from many locations along the famed “tiger stripes” near the south pole of Saturn’s moon Enceladus. Credit: NASA/JPL/Space Science Institute
The Cassini mission has been extended several times since its four-year primary mission was completed on 30 July 2008. The current ‘Cassini Solstice’ mission began in 2010 and is expected to last until 2017.
9 September 1975 – NASA’s Viking 2 spacecraft launched from Cape Canaveral, Florida, bound for Mars. Carried aloft by a Titan-Centaur rocket, Viking 2 comprised an orbiter and a lander segment, same as its sister craft, Viking 1.
The trip to Mars took just shy of a year, arriving on 3 September 1976. The lander segment touched down in Utopia Planitia, which is the largest known impact basin in the Solar System, covering a large swathe of Mars’ northern hemisphere.
The orbiter, meanwhile, sent back over 16,000 images of Mars and one of its two moons, Deimos, over a period of 22 months, before it had to be deactivated following a malfunction in its propulsion system.
Viking 2 lander operated for over three years, concluding on 11 April 1980 when its radioisotope thermoelectric-charged batteries failed.
The twin Viking missions brought us the first images from the surface of Mars, and provided the first direct measurements of the planet’s surface soil composition, as well as testing for signs which could indicate the presence of organic life.